activity
20042017
most citedDetection of 107 glitches in 36 southern pulsars

208 citations · 410 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2017★ 19 cited

Investigating multi-frequency pulse profiles of PSRs B0329+54 and B1642-03 in an inverse Compton scattering (ICS) model

L. H. Shang, J. G. Lu, Y. J. Du +17

The emission geometries, e.g. the emission region height, the beam shape, and radius-to-frequency mapping, are important predictions of pulsar radiation model. The multi-band radio…

astro-ph.HE2012★ 19 cited

Radio and Gamma-ray Pulsed Emission from Millisecond Pulsars

YuanJie Du, GuoJun Qiao, Ding Chen

Pulsed gamma-ray emission from millisecond pulsars (MSPs) has been detected by the sensitive Fermi, which sheds light on studies of the emission region and mechanism. In particular…

astro-ph.HE2012★ 208 cited

Detection of 107 glitches in 36 southern pulsars

M. Yu, R. N. Manchester, G. Hobbs +9

Timing observations from the Parkes 64-m radio telescope for 165 pulsars between 1990 and 2011 have been searched for period glitches. A total of 107 glitches were identified in 36…

astro-ph.HE2012

Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

YuanJie Du, GuoJun Qiao

The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish…

astro-ph.GA2011★ 7 cited

Constraint on parameters of the Inverse Compton Scattering model for radio pulsars

M. Lv, H. G. Wang, K. J. Lee +2

The inverse Compton scattering (ICS) model can explain various pulse profile shapes and diversity of pulse profile evolution based on the mechanism that the radio emission is gener…

astro-ph.HE2011★ 33 cited

Gamma-ray Emission from the Vela Pulsar Modeled with the Annular Gap and Core Gap

Y. J. Du, J. L. Han, G. J. Qiao +1

The Vela pulsar represents a distinct group of γ-ray pulsars. Fermi γ-ray observations reveal that it has two sharp peaks (P1 and P2) in the light curve with a phase separation of…